Suzaku Observation : 405034010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '405034010' / Observation identification string
OBSERVER= 'THOMAS NELSON' / Principal Investigator
OBJECT = 'EG AND ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 11.1550 / planned target R.A.(deg)
DEC_OBJ = 40.6794 / planned target DEC.(deg)
RA_NOM = 1.116800000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = 4.067300000000000E+01 / Declination of target (deci. deg)
PA_NOM = 225.2111 / nominal position angle from north to DETY(deg)
MEAN_EA1= 11.167994020021 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 49.327005655447 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 224.788913504340 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-02-05T15:04:28' / Start date of observations
DATE-END= '2011-02-08T00:04:20' / End date of observations
TSTART = 3.502364670000000E+08 / time start
TSTOP = 3.504386444399957E+08 / time stop
TELAPSE = 2.021774399957061E+05 / elapsed time
ONTIME = 1.005493345608115E+05 / On-source time
EXPOSURE= 1.005493345608115E+05 / Exposure time
MJD-OBS = 5.559766355537037E+04 / MJD of data start time
FILIN001= 'ae405034010xi0_0_3x3n066l_cl.evt.gz' / Input file name
SEQPNUM = 2 / Number of times this dataset processed
PROCVER = '3.0.22.44' / Processing script version
MK1STVER= 'mk1stfits20120530' / Version of mk1stfits used
SOFTVER = 'Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22' / Version of HEADAS used
CALDBVER= 'hxd20110913_xis20160607_xrt20110630_xrs20060410' / Version of CALDB u
FILIN002= 'ae405034010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae405034010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae405034010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae405034010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae405034010xi3_0_5x5n066a_cl.evt.gz' / Input file name
COMMENT -------------------------
COMMENT BITPIX compressed from 32 to 8.
COMMENT Pixel values greater than 255 was set to 255.
COMMENT This file was made for JUDO-Suzaku.
COMMENT -------------------------
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
Abstract:
The goals of this proposal are to use Suzaku XIS observations to : 1) determine whether EG And, BX Mon, and BF Cyg are members of the recently recognized class of hard X-ray emitting symbiotic stars; and 2) if they are, compare the nature of any absorption, the optical depth of the boundary layer, and the accretion rate to those of the well established hard X-ray symbiotics. Understanding the accretion processes in symbiotic stars is a crucial step in determining the role they play as progenitors of type Ia supernovae.